HARMONI at ELT: Modelling the optical performance of a diffraction limited integral field spectrograph

被引:0
|
作者
Todd, Stephen P. [1 ]
Bond, Charlotte Z. [1 ]
Clarke, Fraser [2 ]
Harvey, Eamonn J. [1 ]
Menduina-Fernandez, Alvaro [3 ]
Tecza, Matthias [2 ]
机构
[1] Royal Observ Edinburgh, UKATC, Blackford Hill, Edinburgh EH9 3HJ, Midlothian, Scotland
[2] Univ Oxford, Dept Phys, Denys Wilkinson Bldg,Keble Rd, Oxford OX1 3RH, England
[3] Civil Aviat Author Space Regulat, London E14 4HD, England
来源
MODELING, SYSTEMS ENGINEERING, AND PROJECT MANAGEMENT FOR ASTRONOMY XI, PT 1 | 2024年 / 13099卷
关键词
spectrograph; infrared spectroscopy; diffraction; optical modelling;
D O I
10.1117/12.3019747
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
HARMONI is the first light visible and near-IR integral field spectrograph for the ELT. It covers a large spectral range from 470 nm to 2450 nm with resolving powers from 3300 to 18000 and spatial sampling from 60 mas to 4 mas. It can operate in two Adaptive Optics modes - SCAO (including a High Contrast capability) and LTAO - or with NOAO. To model the optical performance we include manufacturing and alignment tolerances alongside other static and dynamic effects. Diffraction of both image and pupil become significant when the spectrograph slit width matches the diffraction limited point spread function. A set of Zemax OpticStudio macros and Python scripts are used to bring together the subsystem models that make up HARMONI and combine them to include all these effects. We present an overview of our approach to modelling this complex instrument and key results predicting the optical performance of HARMONI.
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页数:13
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